Black Holes at the LHC

dc.creatorDimopoulos, Savas
dc.creatorLandsberg, Greg
dc.date2001-06-27
dc.date.accessioned2026-07-07T10:32:52Z
dc.date.available2026-07-07T10:32:52Z
dc.descriptionIf the scale of quantum gravity is near a TeV, the LHC will be producing one black hole (BH) about every second. The BH decays into prompt, hard photons and charged leptons is a clean signature with low background. The absence of significant missing energy allows the reconstruction of the mass of the decaying BH. The correlation between the BH mass and its temperature, deduced from the energy spectrum of the decay products, can test experimentally the higher dimensional Hawking evaporation law. It can also determine the number of large new dimensions and the scale of quantum gravity.
dc.description5 pages, 3 figures, submitted to PRL. Results presented at the Les Houches Workshop "Physics at the TeV Colliders" (May 30, 2001) and the "Avatars of M-Theory" conference, ITP at Santa Barbara (June 7, 2001), http://online.itp.ucsb.edu/online/mtheory_c01/dimopoulos
dc.identifierhttps://arxiv.org/abs/hep-ph/0106295
dc.identifierhttp://arxiv.org/abs/hep-ph/0106295
dc.identifierPhys.Rev.Lett.87:161602,2001
dc.identifierdoi:10.1103/PhysRevLett.87.161602
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178907
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Experiment
dc.subjectHigh Energy Physics - Theory
dc.titleBlack Holes at the LHC
dc.typetext

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